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Search Results for 'Metallicity Evolution'
Metallicity Evolution published presentations and documents on DocSlides.
How Environment Affects Galaxy Metallicity:
by yoshiko-marsland
Lessons from the. Illustris Simulation . Shy . Ge...
Halo Metallicity in NGC 891
by haroublo
An X-ray/UV Perspective. Edmund Hodges-. Kluck. Jo...
Understanding Metallicity
by joyousbudweiser
at High Redshift Universe. KenTaro. Motohara . (....
Chemical Cartography with SDSS/APOGEE
by trish-goza
Michael Hayden (NMSU), Jo . Bovy. (IAS), Steve ....
Milky Way thin disk
by sherrill-nordquist
Q: in order to study the spatial distribution of ...
HII Region Metallicity Distribution in the Milky Way Disk
by stefany-barnette
Dana . Balser. (NRAO) . Loren Anderson (WVU), To...
Physical Conditions in the ISM
by backbays
Lisa Kewley. Australian National University. Thank...
Assembling the Milky Way
by newson
David Spergel. What has changed?. Context:. Standa...
Probing the first stars with metal poor
by lindy-dunigan
stars. T. . Sivarani. . Indian Institute of Astr...
Chemical Composition of
by test
Planet-Host Stars. 2013. 2. 22. . Wonseok. Kang ...
F-type Stars
by ellena-manuel
“Stars in transition”. Caroline Roberts. Pola...
Long-term project to test effects of
by giovanna-bartolotta
metallicity. on pulsating B stars in the LMC (. ...
50 Years of Wide Field Studies
by briana-ranney
50 years of Wide Field Studies, La Serena, 5/2013...
Stellar populations in disc galaxies from the CALIFA survey
by luanne-stotts
Patricia . Sánchez-Blázquez. (UAM). Jairo. Me...
Molecular Gas in
by tatyana-admore
Low-. Redshift. Galaxies. Adam Leroy (NRAO, Nor...
Dust in Dwarf Galaxies
by ellena-manuel
Adam Leroy. National Radio Astronomy Observatory....
Determining Ages of APOGEE Giants with Known Distances
by pasty-toler
Diane Feuillet . New Mexico State University. Jon...
Maser Discoveries with the SKA
by yoshiko-marsland
Steve . Goldman. 12 April, 2016. Cavendish Labora...
Nuclear Physics and Low-
by lois-ondreau
Metallicity. Stellar Abundances: Victories and S...
understanding
by solidbyte
Ultra Metal - Poor (UMP ; [Fe/H] - 4 . 0 ) stars h...
[C II ] is an important SF tracer in particularly in low-metallicity environments, because of la
by amelia
SOFIA [C . II. ]158 . μ. m vs H . I, . and ...
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